LMC N49

{{Short description|Supernova remnant in the constellation Dorado}}

{{sky|05|26|01.00|-|66|05|06.0|165000}}

{{Infobox nebula

|name = LMC N49

|image = Sig06-030.jpg

|caption =

|credit =

|type = Supernova remnant

|type2 =

|epoch = J2000.0

|subtype =

|class =

|ra = {{RA|05|26|01.00}}

|dec = {{DEC|-66|05|06.0}}

|dist_ly = 160,000

|dist_pc =

|dist_z =

|appmag_v = 12.71

|appdia =

|size_v =

|constellation = Dorado

|radius_ly =

|radius_pc =

|dimensions = 75 ly across

|absmag_v =

|notes =

|names = LMC N49, PKS 0525-66, PKS B0525-661, PKS J0525-6604, SNR J052559-660453

}}

{{commonscat|N49}}

N49 or LMC N49 (PKS 0525-66, PKS B0525-661, PKS J0525-6604, SNR J052559-660453), also known as Brasil Nebula,Sky & Telescope, August 2004, page 12 is the brightest supernova remnant in the Large Magellanic Cloud, approximately 160,000 light-years from Earth. Its form has been assessed to be roughly 5,000 years old.

The latest pictures of N49 by the Chandra X-ray Observatory have revealed a bullet-shaped object traveling at about 5 million miles an hour away from a bright X-ray and gamma-ray point source, probably a neutron star with an extremely powerful magnetic field, known as a soft gamma repeater. A particularly strong gamma-ray burst from LMC N49 was detected on March 5, 1979.

References

{{reflist|refs=

{{cite web |url= http://ned.ipac.caltech.edu/cgi-bin/objsearch?objname=LMC+N49&extend=no&hconst=73&omegam=0.27&omegav=0.73&corr_z=1&out_csys=Equatorial&out_equinox=J2000.0&obj_sort=RA+or+Longitude&of=pre_text&zv_breaker=30000.0&list_limit=5&img_stamp=YES |title= PKS 0525-66 |publisher= NASA/IPAC Extragalactic Encyclopedia }}

{{cite simbad |title= SNR J052559-660453 }}

{{cite web |url= http://chandra.harvard.edu/photo/2010/n49/ |title=N49: Stellar Shrapnel Seen in Aftermath of Explosion |author=Chandra X-ray Observatory |date=2010-05-24 |accessdate=2015-10-15}}

{{cite web |url=http://annesastronomynews.com/photo-gallery-ii/nebulae-clouds/n49-is-a-supernova-remnant-that-spans-about-30-ly-in-the-lmc-a-newly-born-magnetar-a-highly-magnetized-spinning-neutron-star-is-left-over-in-the-ancient-stellar-explosion-which-created-supernova-r/ |title= N49, an asymmetric supernova remnant in the LMC |work= Anne's Astronomy News |date=2012-08-30 |accessdate=2015-10-15}}

}}

  • Harvard-Smithsonian Center for Astrophysics, [https://www.cfa.harvard.edu/ssp/extreme_astrophysics/n49.html "N49: A supernova remnant in the Large Magellanic Cloud"]

{{Dorado}}

{{DEFAULTSORT:LMC N49}}

Category:Dorado

Category:Large Magellanic Cloud

Category:Supernova remnants